HD 114762 b is a small red dwarf star, in the HD 114762 system, formerly thought to be a massive gaseous extrasolar planet, approximately 126 light-years...
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yellow-white F-type main-sequence star (HD 114762 A) and two red dwarf companions (HD 114762 Ab & HD 114762 B) approximately 0.36 & 130 AU distant. Both...
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Pulsar planet (redirect from M62H b)
of the planetary candidate HD 114762 b using Gaia". Astronomy & Astrophysics. 632: L9. arXiv:1910.07835. Bibcode:2019A&A...632L...9K. doi:10.1051/0004-6361/201936942...
51 KB (5,561 words) - 10:31, 2 November 2024
30 Arietis (redirect from HD 16232)
was found to fall in the mass range of red dwarf stars. HD 114762 b HD 114762 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release...
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HD 114762 b: This object has a minimum mass 11 times the mass of Jupiter and has an 89-day orbit. At the time of its discovery it was regarded as a probable...
83 KB (8,227 words) - 13:32, 28 September 2024
2000–2009. HD 114762 b was once considered as the first discovered exoplanet. Found in 1989 by a team led by David Latham, it is now known to be a red dwarf...
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exoplanet research. He is co-discoverer of HD 114762 b, the first substellar mass object (the status of a planet or brown dwarf remains uncertain) known...
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a peculiar star near the nucleus of the Andromeda Galaxy (Messier 31). Latham's planet is the small red dwarf star or massive brown dwarf HD 114762 b...
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Cobalt Blue'". SpaceNews. Retrieved 2024-01-28. "Exoplanet Catalog - HD 189733 b". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2024-01-28...
187 KB (11,623 words) - 15:19, 1 November 2024
Gamma Cephei Ab (redirect from Gamma Cephei b)
γ Cephei Ab to be 9.4 MJ. Dimidium HD 114762 b Iota Horologii b Poltergeist Phobetor "ESA Science & Technology - A brief introduction to exoplanets"....
9 KB (811 words) - 08:18, 5 October 2024